2020
DOI: 10.1140/epjc/s10052-020-8065-9
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Simulation of geodesic trajectory of charged BTZ black holes in massive gravity

Abstract: In order to classify and understand structure of the spacetime, investigation of the geodesic motions of massive and massless particles is a key tool. So the geodesic equation is a central equation of gravitating systems and the subject of geodesics in the black hole dictionary attracted much attention. In this paper, we give a full description of geodesic motions in three-dimensional spacetime. We investigate the geodesics near charged BTZ black holes and then generalize our prescriptions to the case of massi… Show more

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Cited by 21 publications
(11 citation statements)
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References 130 publications
(151 reference statements)
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“…It would be quite interesting to apply the above technique for other spacetimes such as Kerr-de Sitter spacetime [60][61][62], Kerr-Newman-de Sitter spacetimes [63][64][65], charged BTZ black hole [66][67][68] and black holes in Horava gravity [69,70] for defining a global temperature and entropy for these spacetimes.…”
Section: Discussionmentioning
confidence: 99%
“…It would be quite interesting to apply the above technique for other spacetimes such as Kerr-de Sitter spacetime [60][61][62], Kerr-Newman-de Sitter spacetimes [63][64][65], charged BTZ black hole [66][67][68] and black holes in Horava gravity [69,70] for defining a global temperature and entropy for these spacetimes.…”
Section: Discussionmentioning
confidence: 99%
“…taking into account the condition (30). The negative branch is not of our interest, since it has no classical interpretations 2 .…”
Section: General Analysis Of the Equations Of Motionmentioning
confidence: 99%
“…taking into account the condition (30). The negative branch is not of our interest, since it has no classical interpretations.…”
Section: The Evolution Of the Radial Distance (The R -Motion)mentioning
confidence: 99%